Two good-sized coronal holes have rotated around to the center of the sun where they will be spewing solar wind towards Earth were observed by NASA's Solar Dynamics Observatory on Nov. 8-9, 2016.

Two good-sized coronal holes have rotated around to the center of the sun where they will be spewing solar wind towards Earth were observed by NASA's Solar Dynamics Observatory on Nov. 8-9, 2016.
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A bright, flashing eruption on the edge of the Sun was caught in extreme ultraviolet light by the EIT 304 angstrom instrument on SOHO (Solar and Heliospheric Observatory). A spectral line of singly-ionized helium at 304 angstroms shows the state of the solar plasma at roughly 60,000 C. This 'small' event was still several times larger than the Earth.
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On March 29, 2014 the sun released an X-class flare. It was observed by NASA's Interface Region Imaging Spectrograph, or IRIS; NASA's Solar Dynamics Observatory, or SDO; NASA's Reuven Ramaty High Energy Solar Spectroscopic Imager, or RHESSI; the Japanese Aerospace Exploration Agency's Hinode; and the National Solar Observatory's Dunn Solar Telescope located at Sacramento Peak in New Mexico. To have a record of such an intense flare from so many observatories is unprecedented. Such research can help scientists better understand what catalyst sets off these large explosions on the sun. Perhaps we may even some day be able to predict their onset and forewarn of the radio blackouts solar flares can cause near Earth - blackouts that can interfere with airplane, ship and military communications. Read more a href= http //1.usa.gov/1kMDQbO rel= nofollow 1.usa.gov/1kMDQbO /a Join our Google+ Hangout on May 8 at 2 30pm EST a href= http //go.nasa.gov/1mwbBEZ rel= nofollow go.nasa.gov/1mwbBEZ /a
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The Solar Terrestrial Relations Observatory (STEREO) spacecraft Behind observed in the 304 Angstrom wavelength a great deal of solar plasma sliding along the edge of the Sun over a two-day period. These immense structures are generated by magnetic forces rooted inside the Sun.
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This illustration lays a depiction of the sun's magnetic fields over an image captured by NASAs Solar Dynamics Observatory on March 12, 2016. The complex overlay of lines can teach scientists about the ways the sun's magnetism changes in response to the constant movement on and inside the sun. Note how the magnetic fields are densest near the bright spots visible on the sun - which are magnetically strong active regions - and many of the field lines link one active region to another. This magnetic map was created using the PFSS - Potential Field Source Surface - model, a model of the magnetic field in the suns atmosphere based on magnetic measurements of the solar surface. The underlying image was taken in extreme ultraviolet wavelengths of 171 angstroms. This type of light is invisible to our eyes, but is colorized here in gold.
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